Our Sun Notes
The Sun’s Atmosphere Photosphere Chromosphere Corona makes light the most prominent layer Chromosphere thin middle layer; gives off reddish light when the photosphere is blocked during a total eclipse Corona outer layer of the atmosphere can be seen during a total eclipse looks like a white halo
Features of the Sun Sunspots Areas of gas that are cooler than surrounding gases Do not give off as much light Appear as dark spots on the Sun
Features of the Sun Prominences Huge looping eruptions of gas Usually near sunspots Arch out into the outer layers of the sun’s atmosphere
Features of the Sun Solar Flares Explosions of hot gas that occur near sunspots Shoot from Sun’s surface releasing tremendous amounts of energy (equivalent to millions of hydrogen bombs) Largest explosions in the solar system
The Sun’s Affect on Earth Some of the light and heat radiated from the sun reaches Earth. It is either reflected, scattered or absorbed.
The Sun’s Affect on Earth Solar wind - Electrically charged particles sent out from the corona. Move in all directions at very high speeds (400km/sec). Responsible for “tails” on comets.
The Sun’s Effect on Earth Auroras - Referred to as the northern and southern lights. Form when charged particles from the sun hit the Earth’s atmosphere. Particles are directed to the north and south poles by the magnetic field around Earth.
The Sun’s Effect on Earth Magnetic storms - A temporary disturbance in the magnetosphere. Associated with solar flares Solar wind from the sun can cause a magnetic storm. Can last 24-48 hours (or can last for many days).
Effects of Magnetic Storms Long-range radio communication can be difficult or impossible. Global Positioning Systems can be ruined. Satellite orbits can be difficult to control. Electric-power grids can experience voltage surges and cause blackouts. Astronauts and high altitude pilots can be subjected to increased levels of radiation.
How could magnetic storms affect you?
Sun Diagram (NB pg. 97)